From bfd7ae0ce72db0b8c327a986ab50d8792d592ad7 Mon Sep 17 00:00:00 2001
From: hawke <hawke@a4c7b220-a359-4231-b37a-efab6cb7d3ee>
Date: Fri, 3 May 2002 14:41:55 +0000
Subject: This commit was generated by cvs2svn to compensate for changes in r2,
 which included commits to RCS files with non-trunk default branches.

git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinBase/ADMCoupling/trunk@3 a4c7b220-a359-4231-b37a-efab6cb7d3ee
---
 doc/documentation.tex | 30 ++++++++++++++++++++++++++++++
 1 file changed, 30 insertions(+)
 create mode 100644 doc/documentation.tex

(limited to 'doc/documentation.tex')

diff --git a/doc/documentation.tex b/doc/documentation.tex
new file mode 100644
index 0000000..bc570bd
--- /dev/null
+++ b/doc/documentation.tex
@@ -0,0 +1,30 @@
+\documentclass{article}
+
+\begin{document}
+
+\title{ADMCoupling}
+\author{Ian Hawke}
+\date{03/05/2002}
+\maketitle
+
+\abstract{ADMCoupling} 
+
+\section{Purpose}
+\label{sec:aux}
+
+This thorn is completely trivial (there's already more words in the
+documentation than in the code). The point is to allow clean coupling
+of matter thorns and spacetime evolution thorns. By making a spacetime
+thorn (such as BSSN) a friend of ADMCoupling it can know about the
+variables of the matter thorns (such as Whisky) as long as they are
+also friends of ADMCoupling, and then the appropriate stress energy
+tensor terms can be included through the {\tt CalcTmunu} interface.
+This avoids explicit dependencies between the spacetime and matter
+evolution thorns. Note that we need to do the same for certain
+analysis thorns, such as ADMConstraints.
+
+\include{interface}
+\include{param}
+\include{schedule}
+
+\end{document}
-- 
cgit v1.2.3

